This article has an erratum: [https://doi.org/10.1051/0004-6361/201731832e]
Error ellipse resulting from fitting the SED of HD 183915, revealing the strong correlation between Teff and EB−V. The red cross identifies the best fit, predicting EB−V = 0.203 whereas the selective extinction derived from Gontcharov (2012) for that star is EB−V = 0.225 (leading to AV = 0.70).
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